work

Elena.Budnik
1 parent c9cb2857
Showing 10 changed files with 17 additions and 17 deletions Show diff stats
Instrument/AMDA/Voyager1/CRS.xml
Instrument/AMDA/Voyager1/LECP.xml
Instrument/AMDA/Voyager1/MAG.xml
Instrument/AMDA/Voyager1/PLS.xml
Instrument/AMDA/Voyager2/CRS.xml
Instrument/AMDA/Voyager2/LECP.xml
Instrument/AMDA/Voyager2/MAG.xml
Instrument/AMDA/Voyager2/PLS.xml
Instrument/AMDA/Voyager2/PWS.xml
NumericalData/AMDA/Galileo/ephemeris/gll-orb-ca.xml
@@ -5,7 +5,7 @@
     <ResourceID>spase://CDPP/Instrument/AMDA/Voyager1/CRS</ResourceID>
     <ResourceHeader>
       <ResourceName>CRS</ResourceName>
-      <AlternateName> </AlternateName>
+      <AlternateName>Cosmic Ray System</AlternateName>
       <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
       <Description>A </Description>
       <Contact>      
@@ -5,7 +5,7 @@
     <ResourceID>spase://CDPP/Instrument/AMDA/Voyager1/LECP</ResourceID>
     <ResourceHeader>
       <ResourceName>LECP</ResourceName>
-      <AlternateName> </AlternateName>
+      <AlternateName>Low-Energy Charged Particles</AlternateName>
       <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
       <Description>A </Description>
       <Contact>      
@@ -4,8 +4,8 @@
   <Instrument>
     <ResourceID>spase://CDPP/Instrument/AMDA/Voyager1/MAG</ResourceID>
     <ResourceHeader>
-      <ResourceName>Triaxial Fluxgate Magnetometer (MAG)</ResourceName>
-      <AlternateName>MAG</AlternateName>
+      <ResourceName>MAG</ResourceName>
+      <AlternateName>Triaxial Fluxgate Magnetometer</AlternateName>
       <ReleaseDate>2009-05-20T21:10:03Z</ReleaseDate>
       <Description>This experiment was designed to investigate the magnetic fields of Jupiter and Saturn, the solar-wind interaction with the magnetospheres of these planets, and the interplanetary magnetic field out to the solar wind boundary with the interstellar magnetic field and beyond, if crossed. The investigation was carried out using two high-field and two low-field triaxial fluxgate magnetometers. Data accuracy of the interplanetary fields was plus or minus 0.1 nT, and the range of measurements was from 0.01 nT to 2.E-3 T.</Description>
       <Contact>
@@ -4,8 +4,8 @@
   <Instrument>
     <ResourceID>spase://CDPP/Instrument/AMDA/Voyager1/PLS</ResourceID>
     <ResourceHeader>
-      <ResourceName>Plasma Spectrometer (PLS)</ResourceName>
-      <AlternateName>PLS</AlternateName>
+      <ResourceName>PLS</ResourceName>
+      <AlternateName>Plasma Spectrometer</AlternateName>
       <ReleaseDate>2009-05-20T21:10:02Z</ReleaseDate>
       <Description>The plasma investigation made use of two Faraday-cup detectors, one pointed along the earth-spacecraft line and one at right angles to this line. The earth-pointing detector determined the macroscopic properties of the plasma ions, obtaining accurate values of their velocity, density, and pressure. Three sequential energy scans were employed with (delta E)/E equal to 20, 7.2, and 1.8%, allowing a coverage from subsonic to highly supersonic flow. The side-looking Faraday cup measured electrons in the energy range from 5 eV to 1 keV.</Description>
       <Contact>
@@ -4,8 +4,8 @@
   <Instrument>
     <ResourceID>spase://CDPP/Instrument/AMDA/Voyager2/CRS</ResourceID>
     <ResourceHeader>
-      <ResourceName>Cosmic Ray System (CRS)</ResourceName>
-      <AlternateName>CRS</AlternateName>
+      <ResourceName>CRS</ResourceName>
+      <AlternateName>Cosmic Ray System</AlternateName>
       <ReleaseDate>2009-05-20T21:10:14Z</ReleaseDate>
       <Description>This investigation studied the origin and acceleration process, life history, and dynamic contribution of interstellar cosmic rays, the nucleosynthesis of elements in cosmic-ray sources, the behavior of cosmic rays in the interplanetary medium, and the trapped planetary energetic particle environment. The instrumentation included a High-Energy Telescope System (HETS) and a Low-Energy Telescope System (LETS). The HETS covered an energy range between 6 and 500 MeV/nucleon for nuclei ranging in atomic numbers from 1 through 30. In addition, electrons in the energy range between 3 and 100 MeV were measured by this telescope and an electron telescope. The LETS measured the energy and determined the identity of nuclei for energies between .15 and 30 MeV/nucleon and atomic numbers from 1 to 30. The instruments also measured the anisotropies of electrons and nuclei. In addition, electrons in the energy range between 3 and 100 MeV were measured by the electron telescope.</Description>
       <Contact>
@@ -4,8 +4,8 @@
   <Instrument>
     <ResourceID>spase://CDPP/Instrument/AMDA/Voyager2/LECP</ResourceID>
     <ResourceHeader>
-      <ResourceName>Low-Energy Charged Particles (LECP)</ResourceName>
-      <AlternateName>LECP</AlternateName>
+      <ResourceName>LECP</ResourceName>
+      <AlternateName>Low-Energy Charged Particles</AlternateName>
       <ReleaseDate>2009-05-20T21:10:14Z</ReleaseDate>
       <Description>This experiment was designed to study energetic particles in both planetary and interplanetary environments. In the planetary mode, particle sensing occurred with six different solid-state, totally depleted, surface-barrier type detectors. Both coincidence and singles count data were available from two of the detectors. By looking out at a shallow angle from behind the sun shield, measurements were made in regions where particle fluxes were so high as to saturate low-energy detectors. A current mode option was also available for high flux environments. In the interplanetary mode the experiment was equipped with a particle telescope which had solid-state detectors ranging from 2 - 2450 micrometers in thickness. The telescope consisted of two multi-dE/dx x E systems placed back to back in order to use a common all solid-state active anticoincidence shield. The telescope allowed the identification of protons, alpha particles, and heavier nuclei (Z from 3 to 26) in the range from 0.05 to 30 MeV. The combined dynamic range of all the instruments extended from approximately 1.E-5 to greater than 1.E12 particles/(sq cm-s-sr). The energy range covered extended from approximately 10 keV to greater than 11 MeV for electrons and from approximately 15 keV to greater than or equal to 150 MeV for protons and heavier ions. A stepping motor rotated the array of detectors through eight discrete sectors in 45-deg increments, thus allowing a 360-deg scan. For a description of the experiment see Space Science Reviews, 1977, v. 21, pp. 329-354.</Description>
       <Contact>
@@ -4,8 +4,8 @@
   <Instrument>
     <ResourceID>spase://CDPP/Instrument/AMDA/Voyager2/MAG</ResourceID>
     <ResourceHeader>
-      <ResourceName>Triaxial Fluxgate Magnetometer (MAG)</ResourceName>
-      <AlternateName>MAG</AlternateName>
+      <ResourceName>MAG</ResourceName>
+      <AlternateName>Triaxial Fluxgate Magnetometer</AlternateName>
       <ReleaseDate>2009-05-20T21:10:14Z</ReleaseDate>
       <Description>This experiment was designed to investigate (1) the magnetic fields of Jupiter, Saturn, Uranus, and Neptune and (2) the solar-wind interaction of the magnetospheres of these planets with the interplanetary magnetic field out to the solar-wind boundary with the interstellar magnetic field, and beyond, if crossed. The investigation was carried out using two high-field and two low-field triaxial fluxgate magnetometers. Data accuracy of the interplanetary fields was plus or minus 0.1 nT, and the range of measurements was from 0.01 nT to 2.E-3 T.</Description>
       <Contact>
@@ -4,8 +4,8 @@
   <Instrument>
     <ResourceID>spase://CDPP/Instrument/AMDA/Voyager2/PLS</ResourceID>
     <ResourceHeader>
-      <ResourceName>Plasma Spectrometer (PLS)</ResourceName>
-      <AlternateName>PLS</AlternateName>
+      <ResourceName>PLS</ResourceName>
+      <AlternateName>Plasma Spectrometer</AlternateName>
       <ReleaseDate>2009-05-20T21:10:14Z</ReleaseDate>
       <Description>The plasma investigation made use of two Faraday-cup detectors, one pointed along the earth-spacecraft line and one at right angles to this line. The earth-pointing detector determined the macroscopic properties of the plasma ions, obtaining accurate values of their velocity, density, and pressure. Three sequential energy scans were employed with (delta E)/E equal to 29, 7.2, and 1.8%, allowing a coverage from subsonic to highly supersonic flow. The side-looking Faraday cup measured electrons in the energy range from 5 eV to 1 keV.</Description>
       <Contact>
@@ -4,8 +4,8 @@
   <Instrument>
     <ResourceID>spase://CDPP/Instrument/AMDA/Voyager2/PWS</ResourceID>
     <ResourceHeader>
-      <ResourceName>Plasma Wave System (PWS)</ResourceName>
-      <AlternateName>PWS</AlternateName>
+      <ResourceName>PWS</ResourceName>
+      <AlternateName>Plasma Wave System</AlternateName>
       <ReleaseDate>2009-05-20T21:10:14Z</ReleaseDate>
       <Description>This investigation provided continuous, sheath-independent measurements of the electron density profiles at Jupiter and Saturn and will provide similar measurements for Uranus and Neptune. It also gave basic information on local wave-particle interactions required to carry out comparative studies of the physics of the magnetospheres of these planets. The instrumentation consisted of a 16-channel step frequency receiver and a low-frequency waveform receiver with associated electronics. The frequency range for this instrument was from 10 Hz to 56 kHz. This instrument shared the 10-m antennas developed for the planetary radio astronomy investigation.</Description>
       <Contact>
@@ -4,7 +4,7 @@
     <NumericalData>
         <ResourceID>spase://CDPP/NumericalData/AMDA/Galileo/ephemeris/gll-orb-ca</ResourceID>
         <ResourceHeader>
-            <ResourceName>Callisto Flybys</ResourceName>
+            <ResourceName>flybys callisto</ResourceName>
             <ReleaseDate>2015-10-07T14:35:00.000Z</ReleaseDate>
             <Description>Trajectory of Galileo during Callisto flybys. Obtained from NASA/PDS MAG dataset.
                  Available coordinate systems: